ISO spectroscopy of nearby starburst galaxies
1999 ◽
Vol 193
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pp. 745-746
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Keyword(s):
We present spectroscopic mid-IR observations of prominent starburst galaxies obtained with the Short Wavelength Spectrometer onboard the Infrared Space Observatory. The wavelength range accessible by ISO-SWS (2.5–45 μm) contains a large number of emission lines of atomic and molecular hydrogen and several other atomic species. In this paper we discuss the interpretation of the [Ne III] 15.5 μm/[Ne II] 12.8 μm line-ratio, the faint [OIV]25.9 μm line and the pure rotational lines of molecular hydrogen observed in our target galaxies.
1997 ◽
Vol 159
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pp. 333-336
1997 ◽
Vol 178
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pp. 385-388
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1997 ◽
Vol 189
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pp. 89-92
1997 ◽
Vol 178
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pp. 373-384
Keyword(s):
Keyword(s):